A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles
Abstract This study explores the characteristics of wormhole geometries within the framework of symmetric teleparallel gravity, specifically $$\mathcal {F}(\mathcal {Q})$$ F ( Q ) gravity. By integrating holographic and mixed dark energy density profiles, we derive exact solutions for wormholes. The...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2025-05-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-025-14177-y |
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| author | Sourav Chaudhary S. K. Maurya Jitendra Kumar A. Errehymy Nazek Alessa Haleem Abdel Aty |
| author_facet | Sourav Chaudhary S. K. Maurya Jitendra Kumar A. Errehymy Nazek Alessa Haleem Abdel Aty |
| author_sort | Sourav Chaudhary |
| collection | DOAJ |
| description | Abstract This study explores the characteristics of wormhole geometries within the framework of symmetric teleparallel gravity, specifically $$\mathcal {F}(\mathcal {Q})$$ F ( Q ) gravity. By integrating holographic and mixed dark energy density profiles, we derive exact solutions for wormholes. The analysis focuses on the geometrical aspects of these wormholes, employing rotational velocity to formulate the redshift function and using dark energy density profiles to establish the shape function. By selecting specific parameter values, we show that the derived wormhole solutions meet the flare-out condition within an asymptotic background. We also evaluate the energy conditions, with particular emphasis on the null energy condition at the wormhole throat. Our findings indicate that the coupling constant $$\gamma $$ γ significantly influences the violation of energy conditions, especially the null energy condition, accompanied by graphical representations. Additionally, the research examines key features of the wormholes, such as complexity factor, anisotropy, exoticity, and embedding diagrams. |
| format | Article |
| id | doaj-art-a7acc373cb2048c597f248dade3bc623 |
| institution | DOAJ |
| issn | 1434-6052 |
| language | English |
| publishDate | 2025-05-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj-art-a7acc373cb2048c597f248dade3bc6232025-08-20T03:10:32ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-05-0185512210.1140/epjc/s10052-025-14177-yA study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profilesSourav Chaudhary0S. K. Maurya1Jitendra Kumar2A. Errehymy3Nazek Alessa4Haleem Abdel Aty5Department of Mathematics, Central University of HaryanaDepartment of Mathematical and Physical Sciences, College of Arts and Sciences, University of NizwaDepartment of Mathematics, Central University of HaryanaAstrophysics Research Centre, School of Mathematics, Statistics and Computer Science, University of KwaZulu-NatalDepartment of Mathematical Sciences, College of Science, Princess Nourah bint Abdulrahman UniversityDepartment of Physics, College of Science, University of BishaAbstract This study explores the characteristics of wormhole geometries within the framework of symmetric teleparallel gravity, specifically $$\mathcal {F}(\mathcal {Q})$$ F ( Q ) gravity. By integrating holographic and mixed dark energy density profiles, we derive exact solutions for wormholes. The analysis focuses on the geometrical aspects of these wormholes, employing rotational velocity to formulate the redshift function and using dark energy density profiles to establish the shape function. By selecting specific parameter values, we show that the derived wormhole solutions meet the flare-out condition within an asymptotic background. We also evaluate the energy conditions, with particular emphasis on the null energy condition at the wormhole throat. Our findings indicate that the coupling constant $$\gamma $$ γ significantly influences the violation of energy conditions, especially the null energy condition, accompanied by graphical representations. Additionally, the research examines key features of the wormholes, such as complexity factor, anisotropy, exoticity, and embedding diagrams.https://doi.org/10.1140/epjc/s10052-025-14177-y |
| spellingShingle | Sourav Chaudhary S. K. Maurya Jitendra Kumar A. Errehymy Nazek Alessa Haleem Abdel Aty A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles European Physical Journal C: Particles and Fields |
| title | A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| title_full | A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| title_fullStr | A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| title_full_unstemmed | A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| title_short | A study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| title_sort | study on the geometric configuration and stability of wormholes in symmetric teleparallel gravity influenced by dark energy and rotational velocity profiles |
| url | https://doi.org/10.1140/epjc/s10052-025-14177-y |
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